Exposed water ice on the nucleus of comet 67P/Churyumov-Gerasimenko.

Although water vapour is the main species observed in the coma of comet 67P/Churyumov-Gerasimenko and water is the major constituent of cometary nuclei, limited evidence for exposed water-ice regions on the surface of the nucleus has been found so far. The absence of large regions of exposed water ice seems a common finding on the surfaces of many of the comets observed so far. The nucleus of 67P/Churyumov-Gerasimenko appears to be fairly uniformly coated with dark, dehydrated, refractory and organic-rich material. Here we report the identification at infrared wavelengths of water ice on two debris falls in the Imhotep region of the nucleus. The ice has been exposed on the walls of elevated structures and at the base of the walls. A quantitative derivation of the abundance of ice in these regions indicates the presence of millimetre-sized pure water-ice grains, considerably larger than in all previous observations. Although micrometre-sized water-ice grains are the usual result of vapour recondensation in ice-free layers, the occurrence of millimetre-sized grains of pure ice as observed in the Imhotep debris falls is best explained by grain growth by vapour diffusion in ice-rich layers, or by sintering. As a consequence of these processes, the nucleus can develop an extended and complex coating in which the outer dehydrated crust is superimposed on layers enriched in water ice. The stratigraphy observed on 67P/Churyumov-Gerasimenko is therefore the result of evolutionary processes affecting the uppermost metres of the nucleus and does not necessarily require a global layering to have occurred at the time of the comet's formation.

The diurnal cycle of water ice on comet 67P/Churyumov-Gerasimenko.

Observations of cometary nuclei have revealed a very limited amount of surface water ice, which is insufficient to explain the observed water outgassing. This was clearly demonstrated on comet 9P/Tempel 1, where the dust jets (driven by volatiles) were only partially correlated with the exposed ice regions. The observations of 67P/Churyumov-Gerasimenko have revealed that activity has a diurnal variation in intensity arising from changing insolation conditions. It was previously concluded that water vapour was generated in ice-rich subsurface layers with a transport mechanism linked to solar illumination, but that has not hitherto been observed. Periodic condensations of water vapour very close to, or on, the surface were suggested to explain short-lived outbursts seen near sunrise on comet 9P/Tempel 1. Here we report observations of water ice on the surface of comet 67P/Churyumov-Gerasimenko, appearing and disappearing in a cyclic pattern that follows local illumination conditions, providing a source of localized activity. This water cycle appears to be an important process in the evolution of the comet, leading to cyclical modification of the relative abundance of water ice on its surface.

Compositional homogeneity in the fragmented comet 73P/Schwassmann-Wachmann 3.

The remarkable compositional diversity of volatile ices within comets can plausibly be attributed to several factors, including differences in the chemical, thermal and radiation environments in comet-forming regions, chemical evolution during their long storage in reservoirs far from the Sun, and thermal processing by the Sun after removal from these reservoirs. To determine the relevance of these factors, measurements of the chemistry as a function of depth in cometary nuclei are critical. Fragmenting comets expose formerly buried material, but observational constraints have in the past limited the ability to assess the importance of formative conditions and the effects of evolutionary processes on measured composition. Here we report the chemical composition of two distinct fragments of 73P/Schwassmann-Wachmann 3. The fragments are remarkably similar in composition, in marked contrast to the chemical diversity within the overall comet population and contrary to the expectation that short-period comets should show strong compositional variation with depth in the nucleus owing to evolutionary processing from numerous close passages to the Sun. Comet 73P/Schwassmann-Wachmann 3 is also depleted in the most volatile ices compared to other comets, suggesting that the depleted carbon-chain chemistry seen in some comets from the Kuiper belt reservoir is primordial and not evolutionary.

The spectrum of comet Hale-Bopp (C/1995 O1) observed with the Infrared Space Observatory at 2.9 astronomical units from the sun.

Comet Hale-Bopp (C/1995 O1) was observed at wavelengths from 2.4 to 195 micrometers with the Infrared Space Observatory when the comet was about 2.9 astronomical units (AU) from the sun. The main observed volatiles that sublimated from the nucleus ices were water, carbon monoxide, and carbon dioxide in a ratio (by number) of 10:6:2. These species are also the main observed constituents of ices in dense interstellar molecular clouds; this observation strengthens the links between cometary and interstellar material. Several broad emission features observed in the 7- to 45-micrometer region suggest the presence of silicates, particularly magnesium-rich crystalline olivine. These features are similar to those observed in the dust envelopes of Vega-type stars.

A determination of the HDO/H2O ratio in comet C/1995 O1 (Hale-Bopp).

Deuterated water (HDO) was detected in comet C/1995 O1 (Hale-Bopp) with the use of the James Clerk Maxwell Telescope on Mauna Kea, Hawaii. The inferred D/H ratio in Hale-Bopp's water is (3.3 +/- 0.8) x 10(-4). This result is consistent with in situ measurements of comet P/Halley and the value found in C/1996 B2 (Hyakutake). This D/H ratio, higher than that in terrestrial water and more than 10 times the value for protosolar H2, implies that comets cannot be the only source for the oceans on Earth.

Outgassing behavior and composition of comet C/1999 S4 (LINEAR) during its disruption.

The gas activity of comet C/1999 S4 (LINEAR) was monitored at radio wavelengths during its disruption. A runaway fragmentation of the nucleus may have begun around 18 July 2000 and proceeded until 23 July. The mass in small icy debris (

Evolution of the outgassing of comet Hale-Bopp (C/1995 O1) from radio observations.

Spectra obtained from ground-based radio telescopes show the progressive release of CO, CH3OH, HCN, H2O (from OH), H2S, CS, H2CO, CH3CN, and HNC as comet Hale-Bopp (C/1995 01) approached the sun from 6.9 to 1.4 astronomical units (AU). The more volatile species were relatively more abundant in the coma far from the sun, but there was no direct correlation between overabundance and volatility. Evidence for H2O sublimation from icy grains was seen beyond 3.5 AU from the sun. The change from a CO-driven coma to an H2O-driven coma occurred at about 3 AU. The gas outflow velocity and temperature increased as Hale-Bopp approached the sun.

Deuterium in comet C/1995 O1 (Hale-Bopp): detection of DCN.

Deuterated hydrogen cyanide (DCN) was detected in a comet, C/1995 O1 (Hale-Bopp), with the use of the James Clerk Maxwell Telescope on Mauna Kea, Hawaii. The inferred deuterium/hydrogen (D/H) ratio in hydrogen cyanide (HCN) is (D/H)HCN = (2.3 +/- 0.4) x 10(-3). This ratio is higher than the D/H ratio found in cometary water and supports the interstellar origin of cometary ices. The observed values of D/H in water and HCN imply a kinetic temperature >/=30 +/- 10 K in the fragment of interstellar cloud that formed the solar system.

The composition of cometary ices.

The chemical composition of cometary ices provides clues for the conditions of formation and evolution of the early Solar System. A large number of molecules have been identified in cometary atmospheres, from both ground-based observations and space, including in situ investigations. This includes large organic molecules, which are also observed in star-forming regions. This paper presents a review of molecular abundances measured in cometary atmospheres from remote sensing observations with ground-based and space-based telescopes. The diversity of composition observed in comet populations is presented and discussed.This article is part of the themed issue 'Cometary science after Rosetta'.

Cystemustine induces redifferentiation of primary tumors and confers protection against secondary tumor growth in a melanoma murine model.

N'-(2-Chloroethyl)-N-(2-(methylsulfonyl)-ethyl)-N'-nitrosourea (cystemustine) is a chloroethylnitrosourea that has been used in the treatment of human melanoma. Its main antitumor effect is DNA damage to malignant melanocytes. Although unreported at present, other effects may also account for its cytotoxicity, some of them could be more or less delayed with respect to its administration. In this report, we have developed a model of secondary tumor with B16 melanoma in syngeneic C57B16 recipients to investigate the impact of cystemustine treatment of primary B16 melanoma tumors on the fate of secondary implanted untreated tumors. The data presented in this report indicate that cystemustine-treated cells or the administration of cystemustine provoke an important growth delay of primary melanoma tumors, together with an increase in cell pigmentation and cell morphology changes. Data also show that prime treatment induces a dramatic decrease in tumor weight of secondary untreated tumors accompanied by an increase in melanin content and an alteration of cell morphology. Finally, 1H-NMR spectroscopy was performed on treated B16 cells, showing an alteration in the phospholipid derivatives of melanocytes, suggesting subsequent modifications of membrane phospholipid composition. In conclusion, the data highlight two important findings: (a) cystemustine produces modifications other than DNA damage, i.e., cell morphology changes, pigmentation, and phospholipid metabolism alterations, indicating an interference with cell cycle, cell redifferentiation, and proliferation programs; and (b) cystemustine-treated tumors appear to confer a protective effect against the development of secondary untreated tumors that may be mediated by cytokines or an immune response.

Seasonal exposure of carbon dioxide ice on the nucleus of comet 67P/Churyumov-Gerasimenko.

Carbon dioxide (CO2) is one of the most abundant species in cometary nuclei, but because of its high volatility, CO2 ice is generally only found beneath the surface. We report the infrared spectroscopic identification of a CO2 ice-rich surface area located in the Anhur region of comet 67P/Churyumov-Gerasimenko. Spectral modeling shows that about 0.1% of the 80- by 60-meter area is CO2 ice. This exposed ice was observed a short time after the comet exited local winter; following the increased illumination, the CO2 ice completely disappeared over about 3 weeks. We estimate the mass of the sublimated CO2 ice and the depth of the eroded surface layer. We interpret the presence of CO2 ice as the result of the extreme seasonal changes induced by the rotation and orbit of the comet.

Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta.

The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument on board the Rosetta spacecraft has provided evidence of carbon-bearing compounds on the nucleus of the comet 67P/Churyumov-Gerasimenko. The very low reflectance of the nucleus (normal albedo of 0.060 ± 0.003 at 0.55 micrometers), the spectral slopes in visible and infrared ranges (5 to 25 and 1.5 to 5% kÅ(-1)), and the broad absorption feature in the 2.9-to-3.6-micrometer range present across the entire illuminated surface are compatible with opaque minerals associated with nonvolatile organic macromolecular materials: a complex mixture of various types of carbon-hydrogen and/or oxygen-hydrogen chemical groups, with little contribution of nitrogen-hydrogen groups. In active areas, the changes in spectral slope and absorption feature width may suggest small amounts of water-ice. However, no ice-rich patches are observed, indicating a generally dehydrated nature for the surface currently illuminated by the Sun.

Establishment of IPC 227 cells as human xenografts in rabbits: a model of uveal melanoma.

This study was designed in order to evaluate the feasibility of establishing an animal model of human uveal melanoma. IPC227, a cell line established from the biopsy of a patient with a spindle cell ciliary body melanoma, was transplanted into the anterior chamber of the eye in immunosuppressed New Zealand rabbits. In a second step, a tumour fragment from the anterior chamber was implanted transclerally into the posterior choroid. Complete ophthalmological examinations were then performed on the animals. Characteristic growth patterns were noted depending on the location of implantation. In the anterior chamber, diffuse, flat, heavily pigmented tumours appeared 8 days after the injection of the cell suspension that covered the iris and the angle by day 25, with a success rate of 100%. Nodular, lightly pigmented tumours were obtained 6-7 weeks after subchoroidal implantation, with a 25% success rate. Clinical examination, including fundus photography, ultrasound and magnetic resonance imaging, demonstrated the same characteristics as those of human uveal melanoma, confirming the value of this model for the evaluation of new therapeutic and diagnostic methods in the management of uveal melanoma.

In vivo measurement of diffusion and pseudo-diffusion in skeletal muscle at rest and after exercise.

To investigate whether diffusion-related compartmentalization could be observed in skeletal muscle and whether this compartmentalization was affected by exercising, attenuation curves of signal against diffusion weighting were obtained in skeletal muscle of nine healthy volunteers at rest and after an exercise. Fifteen points were obtained for each diffusion curve with diffusion weightings ranging between approximately 0 and 560 x 10(6) s/m2. Data were fitted a biexponential model using three parameters to yield two apparent diffusion coefficients, a long one, ADCL, and a short one, ADCS, together with the fractional volume, fL, associated with the long one. At rest, values of parameters ADCL, ADCS, and fL were 46 x 10(-9) +/- 37 x 10(-9) m2/s, 1.74 x 10(-9) +/- 0.11 x 10(-9) m2/s, and 3.6 +/- 1.3%, respectively. After exercise, these values were 89 x 10(-9) +/- 37 x 10(-9) m2/s (p < .001 vs. rest), 1.94 x 10(-9) +/- 0.13 x 10(-9) m2/s (p < .001), and 5.2 +/- 1.3% (p < .05), respectively. These variations demonstrate significant changes in attenuation curves between rest and postexercise in skeletal muscle and may support an interpretation of the long and the short components in terms of a microvascular and an extra-microvascular compartments.

Simultaneous measurements of diffusion and transverse relaxation in exercising skeletal muscle.

The aim of this study was to compare proton T2 and apparent diffusion coefficient (ADC) variations induced by exercise in skeletal muscle, to provide some more information on the source of their variations. T2 and ADC were measured in the forearm flexor digitorum muscles in 12 healthy volunteers at rest and after an exercise, using a sequence allowing simultaneous measurements of both parameters. At rest, T2 was 30.6 +/- 1.8 ms (mean +/- 1 SD) and ADC was 1.82 +/- 0.11 x 10(-9) m2/s. With exercise, T2 varied by +2.8 +/- 12% (p < .001 vs. rest) and ADC varied by +12 +/- 3% (p < .001). The recovery of T2 after exercise was faster than that of ADC, with half-times of 7 +/- 2 min and of 15 +/- 8 min (p < .01), respectively. It is concluded that both T2 and ADC with exercise are probably different, T2 mostly reflecting changes in water content and ADC reflecting temperature variations.

Experimental evaluation of nonlinearities of small-sized insertable gradient coils.

A phase imaging technique is proposed to map out and quantify gradient nonlinearities of small-sized insertable gradient coils, assuming the whole-body system gradients are highly linear in the domain of interest. The theory is developed and simple equations are derived to allow quantification. It is applied to a 4-loop 18-cm diameter cylindrical gradient coil of optimal design. Experimental gradient nonlinearity maps are obtained for different fields of view. Gradient non-linearities are quantified locally and in regions of interest, showing close agreement with model data.

[Role of arterial hypertension in the cardiac involvement of acromegaly]. / Rôle de l'hypertension artérielle dans l'atteinte cardiaque de l'acromégalie.

Cardiac disease is common in acromegaly. Several mechanisms have been implicated: hypertension, coronary artery disease, valvular heart disease, endocrinopathies including "acromegalic cardiomyopathy". Fifteen consecutive patients with acromegaly, aged 48 +/- 13 years and treated for 4 +/- 5 years, underwent Doppler echocardiography. The patients had no cardiovascular symptoms: 6 had hypertension for 10 +/- 7 years and were compared with a group of 10 control subjects of the same age (48 +/- 17 years). The myocardial mass index (MMI) was higher in acromegaly (110 +/- 32 vs 82 +/- 12 g/m2, p = 0.02), left ventricular enddiastolic dimensions where comparable (48 +/- 7 vs 48 +/- 5 mm, NS) fractional shortening was slightly greater (0.37 +/- 0.04 vs 0.34 +/- 0.04, p = 0.07) as was velocity of shortening (NS) and the ratio of systolic time intervals (NS). The mitral EF slope was decreased (80 +/- 21 vs 101 +/- 30 ms; p less than 0.02); the ratio of the amplitudes of the E and A waves was a little decreased and the isovolumic relaxation phase was increased (92 +/- 13 vs 69 +/- 16 ms; p less than 0.01). Hypertensives (N = 6) had higher MMI (133 +/- 27 vs 94 +/- 24 g/m2, p = 0.02). Normotensive patients had larger isovolumic relaxation periods than control subjects (90 +/- 11 vs 69 +/- 16 ms, p less than 0.05). These results show that in the infraclinical phase, the heart in acromegaly is hypertrophied, not dilated. Hypertension plays a significant role in the development of this hypertrophy. Left ventricular systolic function is normal but diastolic function is impaired.

[Functional imaging of human muscle]. / L'imagerie fonctionnelle du muscle humain.

Medical imaging is now giving access not only to anatomy but also to functions of organs in the human body. Functional imaging may yield a direct appreciation of the function of a given organ, as is the case when measuring ejection fraction of heart with SPECT. Alternately the approach is indirect. This is the case of cerebral functional imaging, either with PET or NMR, where the perfusion increase induced by neuronal activity is detected. Recent developments of NMR, combining imaging and spectroscopy, allow now to detect modification of physiological parameters induced by muscular activity. Indirect detection of muscle activity is very rich in information alternately requiring invasive techniques. Water shifts resulting from intense exercise are detected either from muscle volume increase or water signal modifications, using simple NMR sequences. Then it is easy to identify which muscle is involved in a given protocol. These water shifts, studied in various muscles and several types of exercise protocols, reflect the perfusion increase induced by exercise, and the contribution of metabolic products such as lactate. In some patients with metabolic myopathies a decreased adaptation of perfusion has been detected. Perfusion measurements, previously performed by using venous occlusion plethysmography or radioactive tracers, now benefit from recently developed MR techniques. Oxygenation of muscle may be measured either by spectroscopy of myoglobin, allowing a time resolution of 1 second, or by spectroscopic imaging allowing a spatial resolution of 1-2 cm in a few minutes. Muscle temperature may be non invasively monitored by diffusion-weighted MR. Direct detection of muscle activity is useful only in those muscles that cannot be directly observed. Ultrafast MR imaging may be used to study vocal cords or oculomotor muscles. More interesting is the measurement of contractility, either in myocardium or skeletal muscle, allowed by MR with spin-tagging. Another contribution of MR to muscle studies is the possibility to quantify muscle cross section and muscle volume, in order to normalize strength or metabolism measurements. Sequences using T1 or T2 differences between muscular and adipose tissue allow to quantify the true muscular volume in patients with neuromuscular disorders. Protocols combining several of these parameters by interleaved NMR measurements of perfusion, phosphorylated metabolites, lactate, myoglobin, now open the way to many comprehensive non-invasive pathophysiological studies.

[The control of culicidae in Djibouti town. An experience of 7 years (author's transl)]. / La lutte contre les culicidés dans la ville de Djibouti. Une expérience de 7 années.

The control of culicidae in Djibouti is based first on an antilarval action with suppression of breeding areas and use of Dursban and Abate 5 times a year. Baygon, the use of which is more expensive, is employed for imagicidal control in well delimitated foci.

[The question of endemic malaria in Republic of Djibouti (author's transl)]. / Le problème de l'endémie palustre dans la république de Djibouti.

Since 1973 autochthonous cases of malaria due to P. Falciparum have been reported among local population of French Afars and Issas Territory; 191 cases observed between 1973 and 1976 are recorded. Their monthly distribution and geographical repartition are studied, jointly with the distribution of A. gambiae which has been recently collected in the Territory. This study shows a significant correspondance between the presence of A. gambiae and the malaria cases observed which did not come from neighbouring countries. We may, then, expect the development of small disseminated foci, resulting from the simultaneous introduction of both the parasite and its anopheline vector. This brings about a new epidemiological situation for the Territory.